Mostrar registro simples

Radiating, slowly rotating bodies in general relativity

dc.rights.licensehttp://creativecommons.org/licenses/by-nc-sa/3.0/ve/
dc.contributor.authorMelfo, Alejandraes_VE
dc.contributor.authorNúñez, Luises_VE
dc.contributor.authorPatiño, Albertoes_VE
dc.contributor.authorHerrera Cometta, Luises_VE
dc.date2006-01-26es_VE
dc.date.accessioned2006-01-26T09:00:00Z
dc.date.available2006-01-26T09:00:00Z
dc.date.created1994-02-01es_VE
dc.date.issued2006-01-26T09:00:00Zes_VE
dc.identifier.otherT016300000052/0es_VE
dc.identifier.urihttp://www.saber.ula.ve/handle/123456789/17107
dc.description.abstractRadiating, slowly rotating bodies in general relativity (Melfo, Alejandra; Núñez, Luis; Patiño, Alberto; Herrera, Luis) Abstract We propose a method to obtain axisymmetric, dynamic solutions to the Einstein equations that can represent a radiating collapsing body in slow differential rotation. The method is a generalization of the semi-numeric approach developed but Herrera, Jimenez, & Ruggeri, in 1980, for the spherically symmetric case. Solutions are properly matched to the exterior Kerr-Vaidya metric, and the values of the physically relevant variables (density, pressure, fluid velocity, and energy flux) are obtained inside the matter distribution. As an example of the method, a model based on Schwarzschild interior homogeneous static solution is presented.es_VE
dc.format.extent1455628es_VE
dc.language.isoeses_VE
dc.publisherSABER ULAes_VE
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectDistribuciones autogravitanteses_VE
dc.subjectAstrofísicaes_VE
dc.subjectAstrofísica teóricaes_VE
dc.subjectRelatividad generales_VE
dc.titleRadiating, slowly rotating bodies in general relativityes_VE
dc.typeinfo:eu-repo/semantics/article
dc.description.emailmelfo@ula.vees_VE
dc.description.emailnunez@ula.vees_VE
dc.description.emailpatino@ula.vees_VE
dc.description.emaillherrera@dino.conicit.vees_VE
dc.description.tiponivelNivel monográficoes_VE
dc.subject.centroinvestigacionCentro de Física Fundamental (CFF)es_VE
dc.subject.centroinvestigacionCentro Nacional de Cálculo Científico (CeCalCULA)es_VE
dc.subject.facultadFacultad de Ciencias.es_VE
dc.subject.idiomaIngléses_VE
dc.subject.keywordsEinstein equationses_VE
dc.subject.keywordsGravitational collapsees_VE
dc.subject.keywordsRelativityes_VE
dc.subject.keywordsRotating bodieses_VE
dc.subject.keywordsStellar gravitationes_VE
dc.subject.keywordsSchwarzschild metrices_VE
dc.subject.keywordsStellar modelses_VE
dc.subject.keywordsPhysicses_VE
dc.subject.keywordsGeneral relativityes_VE
dc.subject.tipoArtículoses_VE


Arquivos deste item

Thumbnail
Nome:
1994ApJ677H.pdf
Tamanho:
1.388Mb
Formato:
PDF
Visualizar/Abrir
Thumbnail
Nome:
resumen.htm
Tamanho:
1.090Kb
Formato:
HTML
Visualizar/Abrir

Este item aparece na(s) seguinte(s) coleção(s)

Mostrar registro simples